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Part of the book series: Lecture Notes in Physics ((LNP,volume 596))

Abstract

A noncommutative structure of spacetime induced by quantum effects of gravity is proposed and the implementation of the locality principle on such a space is discussed. Heisenberg’s uncertainty relation

$$ \Delta x \geqslant \frac{\hbar } {{\Delta p}} \geqslant \frac{{\hbar c}} {E}$$

and Einstein’s formula

$$ E = mc^2 $$

imply that measurements at short scales create strong gravitational fields which eventually shield the region of interest by a horizon whose size, in the spherical symmetric case, is given by the Schwarzschild radius \( R = \frac{{2Gm}} {{c^2 }}\). Hence, resolutions of distances which are smaller than the Planck length

$$ \lambda _P : = \sqrt {\frac{{G\hbar }} {{c^3 }}} = 1.6 \times 10^{ - 33} cm$$

seem to be impossible. Therefore, the association of points of some smooth manifold with the localization of events has no operative meaning.

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© 2002 Springer-Verlag Berlin Heidelberg

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Fredenhagen, K. (2002). Quantum Fields and Noncommutative Spacetime. In: Scheck, F., Upmeier, H., Werner, W. (eds) Noncommutative Geometry and the Standard Model of Elementary Particle Physics. Lecture Notes in Physics, vol 596. Springer, Berlin, Heidelberg. https://doi.org/10.1007/3-540-46082-9_14

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  • DOI: https://doi.org/10.1007/3-540-46082-9_14

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  • Publisher Name: Springer, Berlin, Heidelberg

  • Print ISBN: 978-3-540-44071-0

  • Online ISBN: 978-3-540-46082-4

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